Cargando…
ACCRETION PROCESSES IN COSMIC SOURCES: The Atmospheres of Accreting White Dwarfs
A comparison is presented between the physical processes operative in single white dwarfs and the physical processes operative in white dwarfs with donor star companions. The physical properties and accretion physics of the hot accreting components in close interacting binaries is presented. The N/C...
Autores principales: | Sion, E.M., Godon, P. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
2018
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5868958/ https://www.ncbi.nlm.nih.gov/pubmed/29595839 |
Ejemplares similares
-
Dwarf novae and the physics of accretion disks
por: Cannizzo, J K
Publicado: (1996) -
Polarized accretion shocks from the cosmic web
por: Vernstrom, Tessa, et al.
Publicado: (2023) -
Accretion-induced variability links young stellar objects, white dwarfs, and black holes
por: Scaringi, Simone, et al.
Publicado: (2015) -
Large Gas-Phase Source
of Esters and Other Accretion
Products in the Atmosphere
por: Peräkylä, Otso, et al.
Publicado: (2023) -
Accretion processes in star formation
por: Hartmann, Lee
Publicado: (2008)